Vertaisarvioitu artikkeli konferenssijulkaisussa (A4)
Progress on the simulation tools for the SOXS spectrograph: Exposure time calculator and End-to-End simulator
Julkaisun tekijät: Genoni M, Scaudo A, Li Causi G, Cabona L, Landoni M, Campana S, Schipani P, Claudi R, Aliverti M, Baruffolo A, Ben-Ami S, Biondi F, Capasso G, Cosentino R, D'Alessio F, D'Avanzoa P, Hershko O, Kuncarayakti H, Munari M, Pignata G, Rubin A, Scuderi S, Vitali F, Young D, Achren J, Araiza-Duran JA, Arcavir I, Battaini F, Brucalassi A, Bruche R, Cappellaro E, Colapietro M, Della Valle M, De Pascale M, Di Benedetto R, D'Orsi S, Gal-Yam A, Hernandez M, Kotilainen J, Marty L, Mattila S, Rappaport M, Ricci D, Riva M, Salasnich B, Smartt S, Sanchez RZ, Stritzinger M, Ventura H
Toimittaja: George Z. Angeli, Philippe Dierickx
Konferenssin vakiintunut nimi: SPIE Astronomical Telescopes + Instrumentation
Kustantaja: SPIE-INT SOC OPTICAL ENGINEERING, PO BOX 10, BELLINGHAM, WA 98227-0010 USA
Julkaisuvuosi: 2022
Journal: Proceedings of SPIE : the International Society for Optical Engineering
Kirjan nimi *: Proceedings of SPIE: Modeling, Systems Engineering, and Project Management for Astronomy X
Tietokannassa oleva lehden nimi: MODELING, SYSTEMS ENGINEERING, AND PROJECT MANAGEMENT FOR ASTRONOMY X
Lehden akronyymi: PROC SPIE
Artikkelin numero: 121870C
Sarjan nimi: Proceedings of SPIE: the International Society for Optical Engineering
Volyymi: 12187
Aloitussivu: 121870C
Sivujen määrä: 20
ISSN: 0277-786X
eISSN: 1996-756X
DOI: http://dx.doi.org/10.1117/12.2628863
Verkko-osoite: https://doi.org/10.1117/12.2628863
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/176792887
We present the progresses of the simulation tools, the Exposure Time Calculator (ETC) and End-to-End simulator (E2E), for the Son Of X-Shooter (SOXS) instrument at the ESO-NTT 3.58-m telescope. The SOXS will be a single object spectroscopic facility, made by a two-arms high-efficiency spectrograph, able to cover the spectral range 350-2000 nm with a mean resolving power R approximate to 4500. While the purpose of the ETC is the estimate, to the best possible accuracy, of the Signal-to-Noise ratio (SNR), the E2E model allows us to simulate the propagation of photons, starting from the scientific target of interest, up to the detectors. We detail the ETC and E2E architectures, computational models and functionalities. The interface of the E2E with external simulation modules and with the pipeline are described, too. Synthetic spectral formats, related to different seeing and observing conditions, and calibration frames to be ingested by the pipeline are also presented.
Ladattava julkaisu This is an electronic reprint of the original article. |